\begin{table}
  \begin{center}
  \caption{
  Cosmologies implemented in \ccl and observables supported in each of them.
  Note that the only reason why angular power spectra appear not to be supported
  in non-flat cosmologies is that the hyperspherical Bessel functions are
  currently not implemented, although their impact is fairly limited. Likewise,
  number counts power spectra are strictly not supported in the presence of
  massive neutrino cosmologies due to the scale-dependent growth rate that
  affects the redshift-space distortions term, even though the impact of this is
  also small for wide tomographic bins. The halo model can make matter power
  spectrum predictions for all cosmologies except those with $\mu / \Sigma$
  modified gravity, but should not be used for massive neutrino models because
  the current version does not distinguish between the cold matter, relevant for
  clustering, and all matter. Finally, notice that in addition to the support
  for the $\mu / \Sigma$ parameterisation of modified gravity, \ccl can make
  predictions for the growth of perturbations for some modified gravity models
  through a user defined $\Delta f(a)$, and that other extensions are supported
  via integration of external modified gravity codes.\label{tab:cosmo}}
  \begin{tabular}{lccccccc}
\hline\hline
Observable/Model & flat $\Lambda$CDM & $\Lambda$CDM+$K$ & $\Lambda$CDM + $m_\nu$ & $w$CDM & $\Lambda$CDM + $\mu/\Sigma$ MG\\[3pt]
\hline
Distances & \checkmark & \checkmark  & \checkmark & \checkmark & \checkmark \\
Growth  & \checkmark & \checkmark & $X$ & \checkmark  &  \checkmark \\
$P_m(k,z)$ & \checkmark & \checkmark & \checkmark & \checkmark & \checkmark \\
Halo Mass Function & \checkmark & \checkmark & $X$ & \checkmark & \checkmark \\
$C_l$, number counts & \checkmark & $X$ & $X$ & \checkmark & \checkmark \\
$C_l$, weak/CMB lensing  & \checkmark & $X$ & \checkmark & \checkmark & \checkmark \\
Correlation function & \checkmark & $X$ & \checkmark & \checkmark & \checkmark \\
Halo model & \checkmark & \checkmark & $X$ & \checkmark & $X$ \\
\hline\hline
\end{tabular}
\end{center}
\end{table}
